Journal
ADVANCED MATERIALS
Volume 32, Issue 30, Pages -Publisher
WILEY-V C H VERLAG GMBH
DOI: 10.1002/adma.202001054
Keywords
cesium; perovskite solar cells; phase stability; thermodynamic stability
Categories
Funding
- National Natural Science Foundation of China [51902324]
- Major Program of Shandong Province Natural Science Foundation [ZR2018ZB0316]
- Qingdao Key Lab of Solar Energy Utilization & Energy Storage Technology
- National Science Fund for Excellent Young Scholars [51822209]
- Young Taishan Scholar Project of Shandong Province
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The stability issue is still one of the main limitations of the commercialization of perovskite photovoltaics. The mixed cation FA(x)Cs(1)(-x)PbI(3)has shown great promise owing to its improved thermal and moisture stability. However, the study of FA(x)Cs(1)(-x)PbI(3)is concentrated on formamidine (FA)-rich perovskite, whereas cesium (Cs)-rich FA(x)Cs(1)(-x)PbI(3)perovskites are barely studied due to the inevitable phase separation when Cs > 30 mol%. Here, a Cs4PbI6-mediated method is developed to synthesize Cs-rich FA(x)Cs(1)(-x)PbI(3)perovskites. It is demonstrated that Cs(4)PbI(6)intermediate phase has a low Cs cation diffusion barrier and therefore offers a fast ion exchange with the preformed FA-rich perovskite phase to finally form the Cs-rich FA(x)Cs(1)(-x)PbI(3)perovskite. The results indicate that approximate to 15% alloying with organic FA cations can sufficiently stabilize the perovskite phase with excellent phase and UV-irradiation stability. The FA(0.15)Cs(0.85)PbI(3)perovskite solar cells achieve a champion power conversion efficiency of 17.5%, showing the great potential of Cs-based perovskites for efficient and stable solar cells.
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